TESS previously revealed that Thuban, a former North Star, is also a eclipsing binary, as illustrated here. Three such pairs make up a newly discovered sextuple star system called TYC 7037-89-1. Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA)

Name: TYC 7037-89-1

Discovery: TYC 7037-89-1 is the first six-star system ever found where all of the stars participate in eclipses, a discovery made by NASA’s Transiting Exoplanet Survey Satellite. The system is located about 1,900 light-years away in the constellation Eridanus.

Facts: The system, also called TIC 168789840, is the first known sextuple composed of three sets of eclipsing binaries, Stellar pairs whose orbits tip into our line of sight so we observe the stars alternatively passing in front of each other. Each eclipse causes a dip in the system’s overall brightness. Astronomers designate the binaries by the letters A, B, and C. The stars in the A and C systems orbit each other roughly every day and a half, and the two binaries orbit each other about every four years. The B binary’s members circle each other about every eight days, but the pair is much farther away, orbiting around the inner systems roughly every 2,000 years. The primary stars in all three binaries are all slightly bigger and more massive than the Sun and about as hot. The secondaries are all around half the Sun’s size and a third as hot.

This schematic shows the configuration of the sextuple star system TYC 7037-89-1. The inner quadruple is composed of two binaries, A and C, which orbit each other every four years or so. An outer binary, B, orbits the quadruple roughly every 2,000 years. All three pairs are eclipsing binaries. The orbits shown are not to scale. Credit: NASA’s Goddard Space Flight Center

Fun Facts: Astrophysicists are very interested in eclipsing binaries because their structure aids detailed measurements of the stars’ sizes, masses, temperatures, and separation as well as the distance to the system. They can use this information to build better models of star formation and evolution. For example, in the case of TYC 7037-89-1, scientists want to learn more about how the primary and secondary stars across the three binaries developed such similar properties and how the three systems became gravitationally bound.

The paper, “TIC 168789840: A Sextuply-Eclipsing Sextuple Star System,” has been accepted by The Astronomical Journal. A pre-print version is available online.